In general, when introducing the different AGN contributions, ASYM parameter varies very little. However, taking into account previous studies, this parameter is sensitive to noise [1]} and is measured for a smaller sample of galaxies, and therefore in galaxy classification it shall be used in combination with other parameters. In addition to ASYM, we found GINI to be one of the most stable parameters in the case of both early- and late-types, showing variations \(<\)  20% up to the 25% of AGN, which still permits the separation between early- and late-types. GINI has been also suggested to trace well sub-structures in galaxies [2]}, mergers and interacting galaxies [3]}, [4]}, [5]}, strong-lensed galaxies [6]}, [7]}, and to correlate with stellar mass tracing the overall structure of a galaxy better than any other morphological parameter [8]}. However, it has been also shown that GINI depends strongly on the signal-to-noise ratio and the choice of the aperture within which it is measured [9]}, [10]}. In addition to this, we saw that light concentration parameters in general (including CABR, CCON, and M20) are less affected by AGN in early-type than in late-type galaxies, and more stable than SMOOTH parameter which shows higher changes when an AGN is present (although lower when dealing with late-type sources), as shown in Table REF .
